ASTEROIDAL OCCULTATION - REPORT FORM +------------------------------+ +------------------------------+ | EAON | | IOTA/ES | | | | INTERNATIONAL OCCULTATION | | EUROPEAN ASTEROIDAL | | TIMING ASSOCIATION | | OCCULTATION NETWORK | | EUROPEAN SECTION | +------------------------------+ +------------------------------+ 1 DATE (YYYY/MM/DD): 2015/09/05 STAR: 2UCAC 40494885 ASTEROID: Hygiea N°: 10 2 OBSERVER: Name: Peter DELINCAK E-mail: pdlink@astronomy.sk Address: SLOVAKIA, Hviezdoslavova 1971, 022 01 Cadca Phone: +421 915 710 121 Web: www.astronomy.sk 3 OBSERVING STATION: Nearest city: Cadca Station: PDlink Observatory Longitude (DD MM SS.s): E 18 42 09.47 (WGS84) Latitude (DD MM SS.s): N 49 24 15.20 (WGS84) Altitude (m): 680.231m (WGS84) Single|Multiple station: Single +----------------------------+ 4 TIMING OF EVENTS: | | | EVENT REPORTED: POSITIVE | | | +----------------------------+ Event code S: observation Start I: Interruption start D: Disappearance J: Interruption end R: Reappearance B: Blink F: Flash E: observation End O: Other (specify) Personal Equation Substracted: No Comments Event Time (UT) P.E. Acc. Code HH:MM:SS.ss S.ss S.ss S - 03:38:50.000 0.10s : - - - : D - 03:41:12.704 0.10s : R - 03:41:29.370 0.05s : - - - : E - 03:41:43.312 0.05s : Duration : 16.67 +/- 0.15s Mid-event : 03:41:21.037 5 TELESCOPE: Type: Mirror optics Aperture: 400mm Magnification: prime focus (f/5) Mount: EQUATORIAL Motor drive: YES Filter: IR 742nm 6 TIMING & RECORDING: Time source: radio signal DCF 77 => RAD+ Sensor: Watec CCD camera QHY5L-II-M Recording: Begin of record at It=100ms (10 Img/s), end at It=50ms (20 Img/s), uncompressed AVI Recording device: PC W7 32b 7 OBSERVING CONDITIONS: Atmospheric transparency: GOOD Wind: NO Temperature: 11C Star image stability: NOT TOO GOOD Minor planet visible: NO 8 ADDITIONAL COMMENTS: Event data details according to the predictions from IOTA. Predicted event time was 03:41:20 UTC (+/- 3s) for my observing position. Predicted maximum duration was 16.0 seconds with a 0.9 mag drop. Position was 32km from predicted central line in N direction inside the shadow with a probability of 99.1%. Exposure time had to be changed during recording due to light of dawn.